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Neutrino Factory and Muon Collider R&D
Muon Production, Capture and Acceleration R&D directed at Physics with Intense Muon Beams
The Neutrino Factory and Muon Collider Collaboration
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 2
A Bit of History
Since 1995 the Neutrino Factory and Muon Collider Collaboration (a.k.a. Muon Collaboration) has pursued an active R&D program that has focused on muon production, capture and acceleration. Initially the physics emphasis was on muon colliders (both a Higgs Factory and an energy frontier machine). By 2000 the focus of the collaboration had shifted to studying the feasibility of a Neutrino Factory. Recently new ideas in muon ionization cooling have reinvigorated the collaboration's efforts on the investigation of energy frontier muon colliders. I will:
1. Review the physics motivation for our activities2. Describe the Collaboration's program3. Explore the synergy between Neutrino Factory and Muon
Collider facilities both from the point of view of the physics program and the accelerator complex
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 3
NFMCC Mission
To study and develop the theoretical tools, the software simulation tools, and to carry out R&D on the hardware that is unique to the design of Neutrino Factories and Muon Colliders
• Extensive experimental program to verify the theoretical and simulation predictions
NFMCC WEB site: http://www.cap.bnl.gov/mumu/
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 4
Current Organization
R&D Tasks
DOE/NSF
Laboratories/MCOGP. Bond, S. Holmes, J. Siegrist
MUTACR. Kephart
CollaborationSpokespersonsA. Bross, H. Kirk
ProjectManager
M. Zisman
Simul. µCOOL Target MICE
ExecutiveBoard
TechnicalBoard
Collaborating Institutions
Neutrino Factory and Muon Collider Collaboration (NFMCC)
Other
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 5
Collaborating Institutions
US International
National LabsArgonne
BNLFermilabLBNL
Oak RidgeThomas Jefferson
UniversitiesColumbiaCornellIIT
IndianaMichigan State
MississippiNorthern Illinois
PrincetonUC-BerkeleyUC-Davis
UC-Los AngelesUC-Riverside
University of Chicago
National LabsBudkerDESYINFN
JINR, DubnaKEKRAL
TRIUMF
UniversitiesKarlsruhe
Imperial CollegeLancaster
OsakaOxfordPohangTel Aviv
Corporate PartnersMuons Inc*
Tech-X Corporation
*SBIR Funding9 Phase I6 Phase IICurrently 8 FT Ph.D.
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 6
Core Program
Targetry R&D: Mercury Intense Target Experiment (MERIT)
Co-Spokesperson: Kirk McDonaldCo-Spokesperson & PM: Harold Kirk
Ionization Cooling R&D: MuCool and MICEMuCool Spokesperson: Alan BrossMICE Deputy Spokesperson: Mike ZismanUS MICE Leader: Dan Kaplan
Simulations & TheoryCoordinator: Rick Fernow
Muon Collider Task Force*
*@ Fermilab
Physics Motivation
Is Muon Production, Capture and Acceleration R&D worth the investment?
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 8
Evolution of a Physics Program
1. Intense Low-energy muon physics
µ e conversion experiment2. Neutrino Factory
High Energy 10-20 GeVPossible Low Energy 4 GeVoption
3. Energy Frontier Muon Collider
1.5 - 4 TeV+
PRSTAB 2002
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 9
Footprint and the Energy Frontier
ILC0.5 → 1.0 TeV (?)
• The VLHC is the largest machine to be seriously considered to date
Stage 1 – 40 TeV> 2 TeV
Stage 2 – 200 TeV> 10 TeV
73km
ILC
CLICCLIC
3 TeVMuon Facilities
are different
Compact Lepton MachineCLEM (2 TeV) 10
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 11
Low-Energy Muon Physicsµ to e conversion - Mu2e
• Sensitive tests of Lepton Flavor Violation (LFV)
In SM occurs via ν mixingRate well below what is experimentally accessible
Places stringent constraints on physics beyond SM
Supersymmetry– Predictions at 10-15
• Requirement – Intense low energy µ beam
Cooling improves stopping efficiency in target of experiment
Might be an appropriate option for a Mu2e expert.
– Time Scale is issueTest bed for Muon Ionization Cooling for NF and MC with intense µbeam
µ e
NN
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 12
Neutrino Factories
Preliminary Design From the International Scoping Study
• Why a Neutrino Factory?Strong case for precision neutrino program
Very Rich Experimental Program
• Want Very Intense νbeam with well-understood systematics
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 13
Low-Energy NFNeutrino Factory Lite
25-50 GeV 4 GeV
40% CostReduction
ISS Preliminary Design
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 14
3 ν Mixing Model
Is a Neutrino Factory needed in order to fill in the blanks?
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 15
Neutrino Factory- ISS
(3σ, ∆m312=0.0022 eV2)
Best possible reach in θ13 for all performance indicators → Neutrino factory
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 16
Theoretical Indications That θ13 may be small
Projections of the allowed regions from the global oscillation data at 90%, 95%, 99%, and 3σ C.L.
Maltoni et. al. hep-ph/0405172 June 2006
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 17
sin2θ13 Model Predictions
Histogram of the number of models for each sin2θ13 bin.
Albright and Chen, hep-ph/0608137 August 2006
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 18
Neutrino Factory To Build or Not to Build
We Don’t Know –But
There is a Natural Decision Point≈ 2012
After NOvA and T2KIf θ13 not seen
orseen at 3σ
Consider Major Upgrades orNew Facility
In order to make an informeddecision about a New Facility and if the NF plays a role –
Will need a RDR ready at this time (IDS)
This defines the R&D Program
Double Chooz/Daya Bay
FNAL → DUSEL
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 19
Muon Collider - Motivation
Reach Multi-TeV Lepton-Lepton Collisions at High Luminosity
Muon Colliders may have special role for precision measurements.
Small ∆E beam spread –Precise energy scans
Small Footprint -Could Fit on Existing Laboratory Site
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 20
Muon Collider at the Energy Frontier
• Comparisons with Energy Frontier e+e- Collider
For many processes - Similar cross sectionsAdvantage in s-channel scalar production
Cross section enhancement of (mµ/me)2
– ≈ 40,000Beam polarization also possible
Polarization likely easier in e+e-
machineMore precise energy scan capability
Beam energy spread and Beamstrahlhung limits precision of energy frontier (3TeV) e+e-
machinesMuon decay backgrounds in MC do have detector implications, however
3 TeV COM Visible Ecm
CLIC Simulation
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 21
MC Physics - Resolving degenerate Higgs
For larger valuesdiscovery at LHC or gau
of tanβ there is a range of heavy Higgs boson masses (H0, A0) for which e+e- linear collider may not be possible due to suppression of coupling to
ge bosons
Precision Energy ScanCapability
of Muon Collider
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 22
Davide Costanzohep-ex/0105033v2
Key Ingredients of the Facilities
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 24
Needs Common to NF and MC Facility
• Proton Driverprimary beam on production target
• Target, Capture, and Decaycreate π’s; decay into µ’s
• Phase Rotationreduce ∆E of bunch
• Coolingreduce emittance of the muons
Cost-effective for NFEssential for MC
• AccelerationAccelerate the Muons
• Storage Ringstore for ~1000 turns
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 25
But there are Key Differences
Neutrino Factory Muon Collider
• CoolingReduce transverse emittance
ε┴ ~ 7 mm• Acceleration
Accelerate to 20-40 GeV
May be as low as 5-7 GeV
• Storage RingNo intersecting beams
• Bunch Merging
• CoolingReduce 6D emittance
ε┴ ~ 3-25 µmεL ~ 70 mm
• AccelerationAccelerate to 1-2 TeV
• Storage RingIntersecting beams
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 26
Key R&D Issues
High Power Targetry – NF & MC (MERIT Experiment)Initial Cooling – NF & MC (MICE (4D Cooling))200 MHz RF - NF & MC (MuCool and Muon’s Inc)
Investigate operation of vacuum RF cavities in presence of high magnetic fieldsInvestigate Gas-Filled RF cavities
Operation in B field and Beam-Induced EffectsWhile obtaining high accelerating gradients (~16MV/m)
Intense 6D Cooling – MCRFOFO “Guggenheim”Helical Channel Cooling (MANX Proposal)Parametric Resonance Ionization Cooling
Bunch RecombinationAcceleration– A cost driver for both NF & MC, but in very different ways
FFAG’s – ( Electron Model Muon Accelerator - EMMA Demonstration)Multi-turn RLA’s
Storage Ring(s) – NF & MCTheoretical Studies NF & MC
Analytic CalculationsLattice DesignsNumeric Simulations
Note: Almost all R&D Issuesfor a NF are currently under
theoretical and experimental study
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 27
Muon Ionization Cooling
Absorber Accelerator Momentum loss is opposite to motion, p, p x, p y, ∆ E decrease
Momentum gain is purely longitudinal
Large emittance
Small emittance
Longitudinal -Emittance ExchangeTransverse
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 28
NF, Muon Collider - Synergy
Neutrino Factory –ISS Preliminary Muon Collider Schematic
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 29
Additional Technologies Needed for a Muon Collider
• Although a great deal of R&D has been done (or is ongoing) for a Neutrino Factory and is applicable to a MC, the Technological requirements for a Muon Collider are Much More Aggressive
Bunch Merging is requiredMUCH more Cooling is required ( MAKE OR BREAK FOR MC ! )
1000X in each transverse dimension, ≈ 10X in longitudinal
Acceleration to much higher energy (20-40 GeV vs. 1.5-3 TeV)Storage rings
Colliding beamsEnergy loss in magnets from muon decay (electrons) is an issue
Palmer et al:RFOFO RingGuggenheim50-60T Solenoid Channel
Muons Inc.High pressure gas-filled cavitiesHelical Cooling ChannelReverse Emittance ExchangeParametric Resonance Induced Cooling
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 30
6 Dimensional Cooling
RFOFO Ring Guggenheim “Ring”
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 31
Helical Cooling Channel
• Magnetic field is solenoid B0+ dipole + quad + …• System is filled with H2 gas, includes rf cavities• Cools 6-D (large E means longer path length)
6D-MANX ExperimentTo Test
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 32
Extreme µ Cooling -PIC & REMEX
• Parametric-Resonance Ionization Cooling
Drive a ½-integer parametric resonanceHyperbolic Motion
xx’=constant• Reverse Emittance
ExchangeIncrease longitudinal ε in order to decrease transverse ε
Space-Charge Effects Could be Critical
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 33
Low-Emittance Muon Collider (LEMC) Concept
Parameter List:
Ecm = 1.5 TeVPeak L = 7X1034
#µ’s/bunch = 1011
Av Dipole B = 10Tδp/p = 1%β*(cm) = 0.5 (!)
Proton driver:E = 8 GeVPower ≈ 1 MW
ILC AcceleratingStructure Envisioned
Scientific Program
R&D InitiativesTargetry, Muon Cooling, Theory and Simulation
MERIT
Mercury Intense Target
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 36
MERIT –Mercury Intense Target
• Test of Hg-Jet target in magnetic field (15T)• Submitted to CERN April, 2004 (approved April 2005)• Located in TT2A tunnel to ISR, in nTOF beam line• Physics Data Run – Oct-Nov, 2007
Single pulse tests equivalent to 4 MW Power On Target40 Hz @ 24 GeV
Movies of viewport #2, SMD camera, 0.1 ms/frame
37
nozzle A before reaming
ORNL 2006 Nov 28 runs10 m/s
ORNL 2006 Nov 29 run, uprighted imageNozzle C 20 m/s
nozzle A after reaming
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 38
Magnet and Hg Jet system installedin TT2A tunnel at CERN
MuCool
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 40
Muon Cooling: MuCool Component R&D
MuCool201 MHz RF Testing
50 cm ∅ Be RF window
MuCoolLH2 Absorber
Body
• MuCoolComponent testing: RF, Absorbers, Solenoids
RF – High Gradient Operation in High B fieldUses Facility @Fermilab (MuCool Test Area –MTA)Supports Muon Ionization Cooling Experiment (MICE)
MuCool Test Area
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 41
Phase I of RF Cavity Closed Cell Magnetic Field Studies (805 MHz)
• Data seem to follow universal curve
Max stable gradient degrades quickly with B field
• Sparking limits max gradient• Copper surfaces the problem
Grad
ient
in
MV/
m
Peak Magnetic Field in T at the Window
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 42
Next 805 MHz study - Buttons
• Button testEvaluate various materials and coatingsQuick Change over
Tantalum Tungsten Molybdenum-zirconium alloyNiobiumNiobium-titanium alloyStainless steel
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 43
RF R&D – 201 MHz Cavity Design
• The 201 MHz Cavity is now operating tested to design gradient - 16MV/m at B=0 and at B= a few hundred Gauss
Did Not Condition!
Note: This cavity was assembled atTJNL using techniques/proceduresused for SCRF
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 44
Future Tests of 201 MHz Cavity Operation in Magnetic Field
• Need Coupling Coil (2.5T) MICE design
Shown in green schematicallyTHIS IS A CRUCIAL TEST FOR MICE AND FOR NF & MC in general
High Gradient RF operation in a magnetic field
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 45
High Pressure H2 Filled Cavity WorkMuon’s Inc
• High Pressure Test Cell• Study breakdown properties
of materials in H2 gas• Operation in B field
No degradation in M.S.O.G. up to ≈ 3.5T
No DifferenceB=0 & B=3T
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 46
Absorber R&D
• Two LH2 absorber designs are being studied Handle the power load differently
• Also considering LiH (solid) for NF Cooling
Forced-Convection-cooled. Has internal heatexchanger (LHe) and heater – KEK SystemTested @MTA to 25W → 100W
Forced-Flow with external cooling loopMuon Collider
MICE
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 48
Muon Ionization Cooling Experiment (MICE)
MICEMeasurement of Muon Cooling
Emittance Measurement @ 10-3
First Beam January 2008
Beam linecommissioning starts Jan 08
Winter 2008
Spring 2008
Neutrino Factory Decision Point≈ 2012
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 49
Muon Ionization Cooling ExperimentMICE
Beam Diffuser
FocusCoils
LiquidHydrogenAbsorbers
RFCavities
Tracking Spectrometers
MatchingCoils
Radiation shield
Magneticshield
CouplingCoils
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 50
US MICE
• Tracker ModuleSolenoidsFiber ribbonsVLPC System
VLPCs, Cryostats and cryo-support equipment, AFEIIt (front-end readout board), VME memory modules, power supplies, cables, etc
• Absorber Focus Coil ModuleLH2 and vacuum safety windows
Fabrication and QC• RF Module
Coupling Coils (with ICST of Harbin University, China)RF Cavities
• Particle IDCerenkov
Design and Simulation
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 52
Key Simulation Studies
• Muon Capture and Bunch RotationUses “standard” cooling componentsKeeps both µ+ and µ-
• Performance of Open Cell RF latticeMight mitigate problems with high-gradient RF in B field if not solved in RF R&D program
• Full optimization of acceleration scheme for NFPast year spent on International Scoping Study → International Design Study for a NF
Arrive at Reference Design Report• Full simulation and performance evaluation of PIC and REMEX• Complete baseline cooling scheme for a Muon Collider• Acceleration scheme for a Muon Collider• Design of low-beta collider ring
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 53
Acceleration
Dogbone RLA - footprint
-5000
-3000
-1000
1000
3000
5000
-15000 -10000 -5000 0 5000 10000 15000 20000 25000 30000 35000
z [cm]
x [cm]µ+
µ−
µ+
µ−
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 54
NFMCC 5 Year Budget Plan
Base Program funds: remain as in FY06: BNL ($0.9M); Fermilab ($0.6M); LBNL ($0.3M)
Including Base: About $3.6M per year plus supplemental ($400k in FY06)
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 55
Conclusions
• Neutrino FactoryCompelling case for a precision neutrino program exists
With present assumptions Neutrino Factory out-performs other options. However, more is needed before concluding this is the right path
– What the on-going Neutrino Physics program tells us (θ13)– Cost and schedule considerations
The collaboration is making excellent progress on R&D on the major sub-systems
Targetry – MERITMuon Cooling – MuCool and MICEAcceleration Design Studies
– FFAG• Also participating in the EMMA experiment in the UK
– RLAStrong Participation in the recently completed International Scoping Study
Move on to the International Design Study– Goal is to deliver a RDR by 2012
Alan Bross High Energy Physics Advisory Panel Meeting July 14, 2007 56
Conclusions II
• Muon ColliderNew concepts in muon cooling improve the prospects for a multi-TeV Muon Collider
Many new ideas emergingFront-end is the same or similar as that for a Neutrino Factory
Definite Synergies with NF R&DFirst end-to-end muon cooling scenario for a Muon Collider has been developed
• Much more to doDetailed simulation and analysis of cooling designs
Space charge and loading effects particularly important in final stages6D Cooling experiment(s)
– Converge on a preferred cooling schemeAccelerationCollider ring
• The NFMCC will work closely with the Fermilab MCTFMuon Collider Coordination Group
Kirk, Bross, Zisman, Shiltsev, Geer